All Tables

Table 1: Classification values for the halo candidates. Note that WD2359-324 is classified as a halo star despite having c=-1; see text.
Table 2: Classification values for the thick-disk candidates.
Table 3: Effective temperatures, surface gravities, and masses of the halo white dwarfs.
Table 4: Effective temperatures, surface gravities, and masses of the thick-disk white dwarfs. The four coolest stars have higher masses than the rest; however, the masses of the former may have been overestimated (see text).
Table 5: Standard deviation of U, V, W for the 361 SPY thin-disk white dwarfs, $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Soubiran et al. (2003) are shown for comparison.
Table 6: Asymmetric drift $V_{\rm lag}$ and standard deviation of U, V, W for the 27 SPY thick-disk white dwarfs, $V_{\rm lag}$ , $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Soubiran et al. (2003), and Chiba & Beers (2000) are shown for comparison.
Table 7: Standard deviation of U, V, W for the seven SPY halo white dwarfs, $V_{\rm lag}$ , $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Chiba & Beers (2000) shown for comparison.